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dc.contributor.author | Albert, A. | es_ES |
dc.contributor.author | Andre, M. | es_ES |
dc.contributor.author | Anghinolfi, M. | es_ES |
dc.contributor.author | Anton, G. | es_ES |
dc.contributor.author | Ardid Ramírez, Miguel | es_ES |
dc.contributor.author | Aubert, J. -J. | es_ES |
dc.contributor.author | Aublin, J. | es_ES |
dc.contributor.author | Avgitas, T. | es_ES |
dc.contributor.author | Baret, B. | es_ES |
dc.contributor.author | Barrios-Martit, J. | es_ES |
dc.contributor.author | Basa, S. | es_ES |
dc.contributor.author | Belhorma, B. | es_ES |
dc.contributor.author | Bertin, V. | es_ES |
dc.contributor.author | Biagi, S. | es_ES |
dc.contributor.author | Bormuth, R. | es_ES |
dc.contributor.author | Felis-Enguix, Iván | es_ES |
dc.contributor.author | Martínez Mora, Juan Antonio | es_ES |
dc.contributor.author | Saldaña-Coscollar, María | es_ES |
dc.date.accessioned | 2020-11-21T04:31:44Z | |
dc.date.available | 2020-11-21T04:31:44Z | |
dc.date.issued | 2018-12-11 | es_ES |
dc.identifier.issn | 1434-6044 | es_ES |
dc.identifier.uri | http://hdl.handle.net/10251/155443 | |
dc.description.abstract | [EN] One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are important in this context and a reliable way to evaluate this performance is needed. In order to measure the pointing accuracy of the detector, one possibility is to study the shadow of the Moon, i.e. the de¿cit of the atmospheric muon ¿ux from the direction of the Moon induced by the absorption of cosmic rays. Analysing the data taken between 2007 and 2016, the Moon shadow is observed with 3.5¿ statistical signi¿cance. The detector angular resolution for downward-going muons is 0.73¿ ±0.14¿. The resulting pointing performance is consistent with the expectations. An independent check of the telescope pointing accuracy is realised with the data collected by a shower array detector onboard of a ship temporarily moving around the ANTARES location. | es_ES |
dc.description.sponsorship | The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-Allies-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fin Bildung and Forschung (BMBF), Germany; Istituto Naziona-le di Fisica Nucleare (INFN), Italy; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINE-CO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severn Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valencia-na), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. | es_ES |
dc.language | Inglés | es_ES |
dc.publisher | Springer-Verlag | es_ES |
dc.relation.ispartof | The European Physical Journal C | es_ES |
dc.rights | Reserva de todos los derechos | es_ES |
dc.subject | Antares neutrino Telescope | es_ES |
dc.subject | Point like neutrino sources | es_ES |
dc.subject | Moon shadow | es_ES |
dc.subject.classification | FISICA APLICADA | es_ES |
dc.title | The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope | es_ES |
dc.type | Artículo | es_ES |
dc.identifier.doi | 10.1140/epjc/s10052-018-6451-3 | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-1-P/ES/PARTICIPACION DEL IFIC EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-2-P/ES/PARTICIPACION DE LA UPV EN ANTARES Y KM3NET-ARCA%2FORCA/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/ANR//ANR-11-LABX-0060/FR/Origines, Constituants et EVolution de l'Univers/OCEVU/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0005/FR/Université Sorbonne Paris Cité/USPC/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0001/FR/INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE/Amidex/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/FR/Earth - Planets - Universe: observation, modeling, transfer/UnivEarthS/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-3-P/ES/PARTICIPACION DE LA UGR EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//CSD2009-00064/ES/Método de Multimensajeros para la Detección de la Materia Oscura/ | es_ES |
dc.rights.accessRights | Abierto | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada | es_ES |
dc.description.bibliographicCitation | Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, M.; Aubert, J-.; Aublin, J.... (2018). The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope. The European Physical Journal C. 78(12):1-9. https://doi.org/10.1140/epjc/s10052-018-6451-3 | es_ES |
dc.description.accrualMethod | S | es_ES |
dc.relation.publisherversion | https://doi.org/10.1140/epjc/s10052-018-6451-3 | es_ES |
dc.description.upvformatpinicio | 1 | es_ES |
dc.description.upvformatpfin | 9 | es_ES |
dc.type.version | info:eu-repo/semantics/publishedVersion | es_ES |
dc.description.volume | 78 | es_ES |
dc.description.issue | 12 | es_ES |
dc.identifier.pmid | 30872956 | es_ES |
dc.identifier.pmcid | PMC6383875 | es_ES |
dc.relation.pasarela | S\382508 | es_ES |
dc.contributor.funder | A*Midex Foundation | es_ES |
dc.contributor.funder | Agence Nationale de la Recherche, Francia | es_ES |
dc.contributor.funder | Region Ile-de-France | es_ES |
dc.contributor.funder | Generalitat Valenciana | es_ES |
dc.contributor.funder | Université Sorbonne Paris Cité | es_ES |
dc.contributor.funder | Institut Universitaire de France | es_ES |
dc.contributor.funder | European Regional Development Fund | es_ES |
dc.contributor.funder | Instituto Nazionale di Fisica Nucleare | es_ES |
dc.contributor.funder | Ministerio de Economía y Competitividad | es_ES |
dc.contributor.funder | Conseil Régional Provence-Alpes-Côte d'Azur | es_ES |
dc.contributor.funder | Netherlands Organization for Scientific Research | es_ES |
dc.contributor.funder | Département du Var and Ville de La Seyne-sur-Mer | es_ES |
dc.contributor.funder | Bundesministerium für Bildung und Forschung, Alemania | es_ES |
dc.contributor.funder | Centre National de la Recherche Scientifique, Francia | es_ES |
dc.contributor.funder | National Authority for Scientific Research, Rumanía | es_ES |
dc.contributor.funder | Council on grants of the President of the Russian Federation | es_ES |
dc.contributor.funder | Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia | es_ES |
dc.contributor.funder | Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers) | es_ES |
dc.contributor.funder | Universidad Autónoma de Madrid | es_ES |
dc.contributor.funder | Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos | es_ES |
dc.contributor.funder | Ministerio de Ciencia e Innovación | es_ES |
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